When a Period Is Not a Full Stop: Light Curve Structure Reveals Fundamental Parameters of Cepheid and RR Lyrae Stars
The ResonanceChecker program was written to check for resonances between modal oscillations from linear MESA RSP output up to the ninth overtone. The code is a work in progress as the project is still being worked on. PlotterProgram was written to take "Fig4" output from ResonanceChecker and recreate the plot that can be seen in Figure 4 within …
Non Uniform Discrete Fourier Transform applied to OGLE-III Type 1 Cepheid photometry database.
The Cepheid Bias: Resolving the Hubble Tension — Resolving the Hubble Tension via the Temporal Equivalence Principle: Cepheid P-L relation dependence on local gravitational potential, explaining the Hubble tension as a systematic environmental effect.
GEOS data for the O-C of the Classical Cepheid RT Aur (GEOS CIRCULAR CEP4)
Explore a newly developed methodology that could allow us to determine the pulsation and orbit periods of binary Cepheids without using any prior knowledge.
InstabilityStrip is a C++ program written to analyze linear data from MESA's RSP and study variable star's instability strips. Originally called BlueEdge_Plotter as this was the first function the program was fitted for.
Python project to find pulsation period of a cepheid star
Non Uniform Discrete Fourier Transform applied to OGLE-III Type 1 Cepheid photometry database.
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